Dynamics of the CO+ coma of comet 29P/Schwasmann-Wachmann 1. (arXiv:2012.08497v1 [astro-ph.EP])

Dynamics of the CO+ coma of comet 29P/Schwasmann-Wachmann 1. (arXiv:2012.08497v1 [astro-ph.EP])
<a href="http://arxiv.org/find/astro-ph/1/au:+Ivanova_O/0/1/0/all/0/1">O. Ivanova</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Agapitov_O/0/1/0/all/0/1">O. Agapitov</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Odstrcil_D/0/1/0/all/0/1">D. Odstrcil</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Korsun_P/0/1/0/all/0/1">P. Korsun</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Afanasiev_V/0/1/0/all/0/1">V. Afanasiev</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Rosenbush_V/0/1/0/all/0/1">V. Rosenbush</a>

Comet-centaur 29P/Schwassmann-Wachmann 1 was observed in CO+ emission and
contin-uum during 2007-2009 using the 6-m Big Telescope Alt-azimuth at the
Special Astrophysical Observatory of the Russian Academy of Sciences. We
analysed the morphology of the CO+ and dust coma. The distributions of dust and
CO+ ions in the coma are not similar and vary depending on the level of comet
activity. CO+ ions are more concentrated towards the nucleus than the dust
continuum. The column density of the CO+ was derived and found to vary from
3.7*10^9 to 4.3*10^10 ions cm^-2. The production rate of CO+ was estimated to
be from (7.01)*10^24 to (1.15)*10^26 ions s^-1. We discuss possible mechanisms
for the ionization of cometary material and show that impact ionization by
solar wind particles is probably the main ionization mechanism at large
heliocentric distances.

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